{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:UE6VDOFVZSV5UW53HAJ2AUUTCJ","short_pith_number":"pith:UE6VDOFV","schema_version":"1.0","canonical_sha256":"a13d51b8b5ccabda5bbb3813a052931256d630c7bfb8aea23bdbca24bfafc6f9","source":{"kind":"arxiv","id":"0803.1484","version":1},"attestation_state":"computed","paper":{"title":"Strong Near-Infrared Emission Interior to the Dust-Sublimation Radius of Young Stellar Objects MWC275 and AB Aur","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Tannirkulam, E. Pedretti, H. McAlister, J. D. Monnier, J. Sturmann, L. Sturmann, N. Turner, R. Millan-Gabet, T. A. ten Brummelaar, T. J. Harries","submitted_at":"2008-03-10T20:00:08Z","abstract_excerpt":"Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust-destruction radius of Herbig Ae stars MWC275 and AB Aur. Our sub-milli-arcsecond resolution observations unambiguously place the emission between the dust-destruction radius and the magnetospheric co-rotation radius. We argue that this new component corresponds to hot gas inside the dust-sublimation radius, confirming recent claims based on spectrally-resolved interferometry and dust evaporation front modeling."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0803.1484","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-03-10T20:00:08Z","cross_cats_sorted":[],"title_canon_sha256":"6a93b2c5a9e4b5a7e0036066825cc91bc4321fa4d1bc3a8e180540e5cea77ad3","abstract_canon_sha256":"2452cb7dc88dad434d301679de3e26ef2c12cf472c876111956ae9a2cc255de3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:09:47.215004Z","signature_b64":"aCXSpcZmBHyPZ2UM1u2GCYu3VmeF4kbjmEHvVKh2iHvGeyQZo4upIEbgkNBKP3v+3oFwWP0AGrmhPDffGyCKBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a13d51b8b5ccabda5bbb3813a052931256d630c7bfb8aea23bdbca24bfafc6f9","last_reissued_at":"2026-07-04T17:09:47.214566Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:09:47.214566Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong Near-Infrared Emission Interior to the Dust-Sublimation Radius of Young Stellar Objects MWC275 and AB Aur","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Tannirkulam, E. Pedretti, H. McAlister, J. D. Monnier, J. Sturmann, L. Sturmann, N. Turner, R. Millan-Gabet, T. A. ten Brummelaar, T. J. Harries","submitted_at":"2008-03-10T20:00:08Z","abstract_excerpt":"Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust-destruction radius of Herbig Ae stars MWC275 and AB Aur. Our sub-milli-arcsecond resolution observations unambiguously place the emission between the dust-destruction radius and the magnetospheric co-rotation radius. We argue that this new component corresponds to hot gas inside the dust-sublimation radius, confirming recent claims based on spectrally-resolved interferometry and dust evaporation front modeling."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0803.1484","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0803.1484/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"0803.1484","created_at":"2026-07-04T17:09:47.214623+00:00"},{"alias_kind":"arxiv_version","alias_value":"0803.1484v1","created_at":"2026-07-04T17:09:47.214623+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0803.1484","created_at":"2026-07-04T17:09:47.214623+00:00"},{"alias_kind":"pith_short_12","alias_value":"UE6VDOFVZSV5","created_at":"2026-07-04T17:09:47.214623+00:00"},{"alias_kind":"pith_short_16","alias_value":"UE6VDOFVZSV5UW53","created_at":"2026-07-04T17:09:47.214623+00:00"},{"alias_kind":"pith_short_8","alias_value":"UE6VDOFV","created_at":"2026-07-04T17:09:47.214623+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ","json":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ.json","graph_json":"https://pith.science/api/pith-number/UE6VDOFVZSV5UW53HAJ2AUUTCJ/graph.json","events_json":"https://pith.science/api/pith-number/UE6VDOFVZSV5UW53HAJ2AUUTCJ/events.json","paper":"https://pith.science/paper/UE6VDOFV"},"agent_actions":{"view_html":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ","download_json":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ.json","view_paper":"https://pith.science/paper/UE6VDOFV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0803.1484&json=true","fetch_graph":"https://pith.science/api/pith-number/UE6VDOFVZSV5UW53HAJ2AUUTCJ/graph.json","fetch_events":"https://pith.science/api/pith-number/UE6VDOFVZSV5UW53HAJ2AUUTCJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ/action/storage_attestation","attest_author":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ/action/author_attestation","sign_citation":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ/action/citation_signature","submit_replication":"https://pith.science/pith/UE6VDOFVZSV5UW53HAJ2AUUTCJ/action/replication_record"}},"created_at":"2026-07-04T17:09:47.214623+00:00","updated_at":"2026-07-04T17:09:47.214623+00:00"}